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Axion cosmology with long-lived domain walls

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Hiramatsu, Takashi, Kawasaki, Masahiro, Saikawa, Ken'ichi, Sekiguchi, Toyokazu·2013·Journal of Cosmology and Astroparticle Physics

Abstract

We investigate the cosmological constraints on axion models where the domain wall number is greater than one. In these models, multiple domain walls attached to strings are formed, and they survive for a long time. Their annihilation occurs due to the effects of explicit symmetry breaking term which might be raised by Planck-scale physics. We perform three-dimensional lattice simulations and compute the spectra of axions and gravitational waves produced by long-lived domain walls. Using the numerical results, we estimated relic density of axions and gravitational waves. We find that the existence of long-lived domain walls leads to the overproduction of cold dark matter axions, while the density of gravitational waves is too small to observe at the present time. Combining the results with other observational constraints, we find that the whole parameter region of models are excluded unless an unacceptable fine-tuning exists.

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Metadata

Authors
Hiramatsu, T., Kawasaki, M., Saikawa, K., & Sekiguchi, T.
Venue
Journal of Cosmology and Astroparticle Physics
Published
2013-01-02
Volume
2013
Issue
01
Pages
001-001
ISSN
  • 1475-7508 (ISSN-L)
  • 1475-7516
OpenAlex
W2139621994
Cited by
158
References
0
FWCI
4.64
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: Axion cosmology with long-lived domain walls. https://app.cochat.ai/papers/10.1088/1475-7516/2013/01/001
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Hiramatsu, T., Kawasaki, M., Saikawa, K., & Sekiguchi, T. (2013). Axion cosmology with long-lived domain walls. Journal of Cosmology and Astroparticle Physics. https://doi.org/10.1088/1475-7516/2013/01/001

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.